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Report written:October 15, 1.954
Work done by:——R. B. 13eysterL. CranbergR. B. DayR. L. lienkelR. L. MillsR. A. NoblesT. R. RobertsR. K. SmithS. G. SydoriakR. G. TaylorM. Walt
... . . . ......-
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UNCLA$ISIFIED\<
LOS ALAMOS SCIENTIFIC LABORATORY
of the
UNIVERSITY OF CALIFORNIA
._ .
LA-1853 This document consists of& p~es -,:
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-. LTOTAL NEUTRON CROSS SECTION OF He3
. .-
PHYSICS AND MATHEMA TICS(M-3679, 15th edition)
mnni
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I PHYSICS AND MATHEMATICS(M-3679, 15th edition)
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1-20212223242526-30313233-3536373839-41424344-4546-515253545556575859-61626364-676869-7677-7879608182-858687-8889909192-939495969’7.99100101102103104-107108109110111112113114115116-118119-121122-123124125126-129130131-145
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ABSTRACT
The total neutron cross section of He3 has been measured over the
energy range from 200 kev to 22 Mev in good geometry. The main feature
of the curve is a maximum at 2 Mev, superimposed on a decrease in cross
section that is otherwise monotonic with increase in energy. Where the
known He3(n, p)T cross section overlaps these measurements, it comprises
about one-third of the total cross section and has a similar variation with
energy. The total elastic scattering cross section is obtained from the
difference bel.ween the total cross section and the (n, p ) cross section for
neutron energies from 600 kev to 4 Mev.I
-3--.—.
——
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1. Introduction
Elecause of3
with He can be
the very strong bhdlng of the last nucleon
interpreted in terms of the characteristics
4in He , the interaction of neutrons
of the alpha particle at high ex-
citatiorm, i. e. , from about 20.5 Mev to about 35 Mev for the range of these measurements.
‘I’he compound states formed by the scattering of neutrons from He3 3and H are two mem-
bers oi an isotopic spin triplet, with T ~ . 0 and Tz = +1, respectively. The third, with
T ~ = -1, corresponds to protons incident on He3, or excited states of Li4. It should be of
interest to compare the properties of the members of this triplet because of their bearing on
the charge independence of nuclear forces. This triplet has the unique property that in ad-
dition to the substitution of an n-n for p-p bond (the property of mirror nuclei), there is one
n-p bond substituted for one n-n or p-p bond. The total scattering cross section is obtained
from the difference between the total cross section and what is known of the total reaction
cross section. No direct measurements of the elastic scattering of neutrons from He3 have
been reported as yet.
These measurements may be regarded as part of an informal program of fundamental
nuclear measurements of the very light nuclides
hers of the Los Alamos Scientific Laboratory in
cilitated by access to large quantities of H3 and
which have been carried out by various mem-
recent years, a program which has been fa-
He3.
2. Method and Procedure
The total cross section of He3 for monoenergetic neutrons has been calculated from the
results of a measurement in good geometry of the neutron transmission T of a vessel filled
with He3, according to the
where N is the number of
section to be determined.
formula
He3 nuclei per
The vessel. was cylindrical, 1 meter
T . e-No
square centimeter of sample, and u is the cross
long, 7/8 inch i. d., with a l/16-inch wall, welded
end-cups 0.100 inch thick, a filling line of flexible capillary tubing, and double valves, all of
stainless steel. A detailed description of the design and testing of the vessel is to be found1in a report by R. L. Mills and F. Edeskuty. This cell was used earlier for the measure-
2ments of the total neutron cross section of tritium.
FUling of the vessel and subsequent recovery of the He3 were carried out by T. R.
Roberts. An account of this work is given in Appendix A.
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Determinations of the number of nuclei per square centimeter of the sample were car-
ried cut by PVT measurements and by weighing, together with a mass-spectroscopic analysis
of the sample. This work was done by Roberts and Mills. A report by Mills describing the
work is given in Appendix B. The filling pressure was 1450 psi, corresponding to 1.47 moles
of He:]. The impurities were less than 0.4 per cent of the number of He3 moles.
Monoenergetic neutrons were generated by the large Van de Graaff, using the reaction
T(p, n)He3 for the neutron energy range from 0.14 to 4.25 Mev. For the range from 4.25 to
8.03 Mev the reaction J3(D, n) Hea was used, and for the range from 14.2 to 21.4 the reaction
was T(D, n) He4. Tn all cases gas targets were used, sealed off with l/20-mil nickel foil.
The target-to-detector distance was 152 cm, with the gas vessel midway between them.
The detector was a stil,bene scintillator, 3/4 inch in diameter and 1 1/2 inches long, coupled
to a Dumont 6467 photomultiplier, which was followed by a linear amplifier and scaler. The
same detector system was used for all the data; only the amplifier gain, photomultiplier volt-
age, and scaler bias were changed with energy.
:Backgrounds were taken with a copper bar 24 inches long in place of the cell, and with
the target evacuated. The amplifier gain and scaler bias were set so that the counting rate
with the copper bar in place was 1 per cent or less of the counting rate without the
flux with sample out was taken with a dummy evacuated cell in lieu of the sample.
Sufficient counts were taken to assure an over-all rms error of not more than
in the transmission.
3. Results
bar. The
1 per cent
The cross sect ions obtained as a function of energy are summarized in Table 1, in curve
1 of Fig. 1 on a log-log scale, and in Fig. 2 on a linear scale. The neutron energies given
correspond to the average energy of a neutron generated in the gas target. The spread in
neutron energy given in
thickness of the target.
tron energy, except for
tector and the shape of
Table 1 is due to the target thickness and corresponds to half the
This spread is to be interpreted as half the effective spread in neu-
the two lowest energy points. At those energies the bias of the de-
the yield curve discriminated against the lower-energy neutrons, so
that the spread in effective energy is less than the spread in neutron energy, perhaps only
two-thirds as much.
The observed transmissions range from 0.44 to 0.83. The uncertainty in the cross
section associated with the 1 per cent standard error of the transmission, which is due to
statistical uncertainty, is 2 per cent for the lowest transmission and 5 per cent for the highest.
Other sources of uncertainty in the cross-section including effect of He3 impurities, uncertainty
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TABLE 1
TOTAL NEUTRON CROSS SECTION OF He3 AS A FUNCTION OF ENERGY
En,
Mev
0.14
0.28
0.39
0.505
0.’736
0.955
1.17
1.39
1.60
1.77
2.02
2.22
2.42
2.63
2.83
3.04
3.23
3.44
3.64
3.84
4.05
A,En,
Mev
*CI.050
+0.040
*0.050
*0.047
+0.042
*0.038
*0.035
*0.032
+0 .030
*0.027
*0.025
&O.023
*0.021
*0.021
*0.020
+0.019
*0.019
*0.018
+0.018
*0.018
*0.017
at’barns
3.44
3.12
2.92
2.82
2.75
2.85
2.95
3.09
3.20
3.20
3.23
3.28
3.08
3.06
2.97
2.95
2.85
2.86
2.74
2.66
2.57
-6-
En,
Mev
4.25
4.85
5.44
5.97
6.50
7.00
7.52
8.03
14.8
16.0
16.9
17.6
18.2
18.8
19.3
19.9
20.4
20.9
21.4
AEn,
Mev
+0.016
*O.1OO
*0.075
+0.063
*0.057
*0.052
*0.046
*0.035
*0.250
*0.400
*0.200
*0.120
+0.090
*0.075
*0.060
*0.055
*0.050
ko.045
*00040
at’
barns
2.58
2.40
2.28
2.19
2.04
2.01
1.90
1.86
1.14
1.04
1.02
0.96
0.88
0.93
0.88
0.87
0.87
0.88
0.81
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in the dimensions and contents of the cell, and inscattering by the sample, are estimated to
have a combined effect not greater than 1 per cent at any cross section. The sum of the
statistical and miscellaneous uncertainties at each energy is very close to 0.06 barns.
The most noteworthy feature of the results is the broad maximum centered at 1.9 + 0.2
Mev, superimposed on a decrease that is monotonic with increasing energy. The general shape
is similar to that which has been found by Coon et al.2 for the total cross section of tritium,
that is, a broad maximum in the Mev region, followed by a smooth drop at higher energies.
At low energies the He3 cross section increases, presumably because of the large He3(n, p )T
contribution to the cross section at the lower energies.
hi the region up to 4.35 Mev neutron energy, the only reactions of neutrons with He3
energetically possible are elastic scattering, radiative capture, and the (n, p ) reaction. If,
following Flowers and Mandl,3 it is assumed that the cross section for He3(n, y)He4 is of the
same order of magnitude as T(p, y)He4, that is, of the order of 10-28 cm2, then the difference
between the total neutron cross section and the (n, p ) reaction cross section is essentially the
elastic scattering cross section.
Curve 2 in Fig. 1 is an extrapolation on a I/v basis of the total cross section for He3
from measurements at thermal and subthermal energies by King and Goldstein.4 This extra-
polation provides a rough estimate of that part of the total cross section due to the (n, p ) re-
action. A more reliable estimate of the latter can be obtained from the principle of detailed
balance by using the results of Jarvis et al.5 and Willard et al.6 for the inverse reaction
T(p, n)He3. These are given as curves 3 and 4, respectively, of Fig. 1. In the case of
Willards data, only that part of the results which corresponds to the experimental points is
used. ‘The extrapolation to threshold is presumed in error because it does not have the cor-
rect slcjpe at threshold and corresponds to a decrease in the (n, p ) reaction cross section with
decrease in energy. A lhird set of data taken at this Laboratory with improved background
determinations corroborate Willards’s results.6 The discrepancy between Jarvis et al. and
Willard et al. is therefore to be resolved in favor of the latter. Direct data on the reaction8cross section obtained by Coon are consistent with the data of curves 3 or 4.
.The difference between the total neutron and the Hes (n, p ) T cross sections is given in
Fig. 3, curve 1, using Willard’s data. For comparison, curve 2 of Fig. 3 gives the curve of
total neutron cross section for tritium as measured by Coon, Bondelid, and Phillips.2 This
is reasonably certain to be entirely due to elastic scattering up to the threshold
8.34 Mev.
At 4.36 Mev, the reaction lIe3(n, D )D becomes possible.
Keyser$t on the inverse reaction, and the principle of detailed
From the data of
balance, the (n, d)
for T(n, 2n)D,
McNeil and
reaction
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accounts for 0.004 barn at a neutron energy of 4.50 Mev. From Hunter and Richards10
data
and detailed balance, the (n, d) reaction accounts for 0.097 barn at 6.4 Mev neutron energy,
or about 5 per cent of the total. It seems likely that above 4.35 Mev the (n, p ) reaction con-
tinues to account for an appreciably larger percentage of the total cross section than this, so
that further data on the He3(n, p )T reaction are necessary to extend knowledge of the elastic
cross section.
It is noteworthy that the reaction and total cross sections have maxima at the same
energy, within experimental error, and, have similar general shapes down to 400 kev. Their
ratio varies smoothly from 0.38 to 0.22, with increasing energy. It is interesting, too, to3 3
note that the peak cross sections for elastic scattering of neutrons from H and He are
equal within the over-all uncertainty of about 0.1 barn. The energies at which the maxima
occur differ by about 2 Mev.
4. Discussion
at 2 Mev may be interpreted
resonance of about 2.6 barns,
interpretation has been placed
The only theoretical interpretation of these data made thus far is by J. Gammel. He
has suggested, tentatively, that the maximum in the scattering
as a p-wave resonance with J = 2. This gives a maximum at
compared to the experimental value of 2.45 barns. The same
on the maximum of the tritium results.
The results on the elastic scattering are of interest in comection with the frequently
made suggestion that the He3(n, p )T reaction be used as a neutron spectrometer. 11The chief
source of background in such an instrument arises from elastic scattering, and these data pro-
vide a basis for estimating quantitatively the importance of this background.
I
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APPENDIX A
He3 CELL FILLING AND RECOVERY
By T. Roberts
The gas vessel was filled with He3, using a modification of the cryogenic pump technique
described by Mills and Edeskutyl in connection with the tritium filling of the same vessel.
The main difference was that the He3 was supplied in 12-liter cans at an average pressure
of about 400 mm Hg instead of uranium pots. In order to condense most of the He3 into the
pump, the surrounding He4 bath was cooled by pumping to about 1.2°K, at which temperature
the vapor pressure of He3 is about 20 mm.
The high-pressure filling line and glass vacuum line were similar to those shown in
Figs. ~, and 7 of Mills nnd Edeskuty, 1 which are reported here as Figs. 4 and 5. The pres-
sure gauge was a Heise O to 5000 psi gauge filled with mercury to reduce dead volume. A
diffusion pump was comected to the high-pressure gauge manifold by only one autoclave valve
in order to increase the pumping speed. The nine He3 tanks furnished by LASL Group CMR -4
were interconnected by a low-pressure manifold of l/8-inch copper tubing and were also con-
nected to the main manifold by a high-pressure valve.
The cryogenic pump was designed to withstand 86001;!
tions. The pump had a volume of 87 cc and was made
piece of 2 l/2-inch round 321-stainless steel stock. The
psi, according to ASME specifica-
by drilling a 1 l/2-inch hole in a
plug had 1 3/4 standard fine threads.
High-pressure tubing 1/4 inch o.d., 3/32 inch id. , was used for the pump inlet tube to pre-
vent the likelihood of air or tritium plugs. In order to warm the cryogenic pump to room
temperature quickly, a l.00-watt wire-wound resistor was taped to the pump.
The pump was pressure tested for 16 hours at 8600 psi and the pump, gauge, and high-
-pressure cell were tested for 60 hours at 1800 psi. To the limit of detectability, about
0.3 per cent, there was no loss in pressure in either experiment.
The only difficulties encountered concerned the sticking of valves on two He3 tanks. It
had been hoped, on the basis of labeled tank contents, that the cell could be filled to 1500 psi
or more, but one tank u’as found to be empty, apparently because the valve stuck shut during
the filling by Group CMR -4. The valve on another tank failed to open during the condensation,
so that 1452 psi at a cell temperature of 28.5°C, was the maximum pressure that could be
achieved.
The He4 dewar contained about 5 1/2 liters, 3 1/2 of which were used up in pumping
the He<Lbath down to 1.2°K and in condensing the He3. Condensation was stopped when the
storage-can pressure had fallen to 55 mm.
-12--.
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The empty He3 tank was useful in the recovery operation. After the cell filling, the
cryogenic pump and high-pressure manifold were bled down to 14 mm pressure by a two-stage
expansion, first, into two of the tanks whose pressure was 55 mm, and then into the empty
tank. The high-pressure manifold was then emptied with the Toepler pump.
After the cross-section measurements, the cell was reconnected to the high-pressure
manifold and the pressure measured as 1441 psi at 27.9°C. The pressure drop was completely
accounted for by the temperature change and the expansion into the empty manifold. The cell
was then emptied to 500 mm pressure by expansion into seven of the tanks and a sample
taken for mass spectrometer analysis. The cell contents then were expanded into the nearly
empty tank to 32 mm and the remaining gas removed by Toeplering for three days.
-15-.—..—.,. .~-——_ .__ .._.. .._-c ...-4
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APPENDIX B
He3 CELL CONTENT
By R. L. Mills
The total charge in the cell was computed by PVT relationships as indicated in Table 1
and from weight changes as shown in Table 2. Results of the mass-spectrographic analysis
of the gas sample are entered in Table 3.
TABLE 1
CELL CONTENT AS DETERMINED BY PVT
Pressure, Volume, Temperature, Cell Content,atm cc oK moles
98.80 * 0.10 384.220 * 0.077 301.6 + 0.1 L468(a)
1.470(b)
1.468(C)
1.470(d)
average 1.469 + 0.002
(a)Co reputed from the virial equation
pv = RT [1 + B(T)/v]
using a value for B(T) determined from the equation
B = (l{T) 1/4 [16.4873 - 74.09( 1/T) ’/2 - 24.6(1/T)] cc/g
as given by F. G. Keys, Temperature, pp. 45-59, Reinhold Publishing Corporation, New York,
1941.
(b)Computed from the virial equation using for B(T) the value 11.38 cc/mole, interpolated
from data rep,orted by W. H. Keesom, Helium, Table 205, p. 38, Elsevier Publishing Company,
Amsterdam, 1942.
(c)Computed from A. C. Johnson’s equation of state
PV = 24875.08 + 11.802p - 0.()() 1094pz cc atm/mole at KIOC
and corrected to 28.5° C. See “IV - Vapor Pressure, Specific Volume, PVT Data for H2, N2,
02, CO, C02, Air, He, A, Hg,” by S. Gratch, Trans. ASME, ‘Q 635 (1948).
(d)Computed from an interpolation of data reported by R. Weibe, V. L. Gaddy, and Conrad
Heins, Jr., “The Compressibility Isotherms of He from -70 to 200° and at Pressures up to
1000 atm,” J. Am. Chem. Sot., 53, 1721 (1931).
-16-
.. . .
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—.
CELL
Wt. Cell FullMinus Tare, g
4.476
TABLE 2
CONTENT AS DETERMINED BY WEIGHT DIFFERENCE OF CELL
Wt. Cell EmptyMinus Tare, g
0.017
—(a) Based on an “average molecular weight”the mass-spectrographic data of Table 3.
Wt. of Gasin Cell, g
4.459 * 0.005
of 3.0685 for the gas
‘b ‘Assuming pure He3 with molecular weight 3.0170.
TABLE 3
MASS SPECTROGRAPHIC ANALYSIS
Symbol Mass h’umber
He3 3
‘228
‘22
HT 4
‘2 6
HD 3
DT 5
Computed. cell contents in Tables 1 and 2 do not
OF CELL
Cell Content,moles
1.453 * o.oo2(a)
1.478 + 0.002(b)
mixture, as computed from
SAMPLE
Mole %
99.62
0.20
0.05
0.05
0.04
0.02
0.02
agree within the combined experimental
errors. Such a discrepancy could easily arise if the gas sample analyzed in Table 3 was not
truly representative of the cell content. For this reason the results of Table 1 have been used
to compute the following concentrations, where L, the cell length, is 99.981 + 0.005 cm, and
N, Avogadro’s number,23
is taken as 6.0228 + 0.0011 x 10 :
(n/V)
(L) (n/V)
(N)(L) (n/V)
(0.9962 )(N)(L) (n/V)
(0.0020 )(N)(L) (n/V)
= 0.003823 * 0.000005 mole/cc
= 0.3822 * 0.0005
= 2.302 * 0.003 X
= 2.293 * 0.003 X
= 0.0046 X 1023
2mole/cm
~023molecules/cm2
~023molecules He3/cm
2
molecules N2/cm2
-17-—_L-—---- __
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1. R. L. Mills and I?. Edeskuty,
2. J. H. Coon, R. Bondelid, and
3. B. H. Flowers and F. Mandl,
References
LAMS-141 1, August 1952 (not available).
D. Phillips, LA-1483, November 1952.
Proc. Roy. Sot. London, A206, 131 (1951).
4. L. D. P. King and L. Goldstein, Phys. Rev., 73, 1366 (1949).
5. ,Jarvis, Hemmendinger, Argo, and Taschek, Phys. Rev., ‘@ 929 (1950).
6. H. B. Willard, J. K. Bair, and J. D. Kington, Phys. Rev., 9A, 865 (1953).
7. IG. A. Jarvis, private communication.
8. J. H. Coon, Phys. Rev., 80, 488 (1950).
9. ‘K. G. McNeil and G. M. Keyser, Phys. Rev., 8Q, 602 (1951).
10. IG. T. Hunter and H. T. Richards, Phys. Rev., ~, 1445 (1945).
11. ;R. Batchelor, Proc. Phys. Sot. London, A65, 674 (1952).
12. “Unfired Pressure Vessels, Section VII I, ASME Boiler and Pressure Code, 1952.
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